横航向驾驶员诱发振荡研究及地面模拟验证

本文建立了包括非线性环节在内的横航向驾驶员—操纵系统—飞机本体组合系统的数学模型,采用闭环控制原理,对JJ-7飞机横航向驾驶员诱发振荡PIO问题进行了研究,并详细地讨论了驾驶员参数及其各种操纵动作、操纵系统和飞机本体气动参数对横航向PIO的影响,探讨了横航向PIO产生的机理。文中以JJ-7飞机为例,采用时域法在整个飞行包线各点进行了检查,并用固基飞行模拟器进行模拟验证。其结果与理论计算结果相一致。     

超声振动体的耦合振动研究

对一些典型的大尺寸超声振动体如圆柱体、空心圆柱体、长条形六面体和大矩形六面体。本文用通用有限元软件对耦合系数的分布进行了分析，并在耦合振动频率方程的基础上研究了耦合系数与耦合振动的强度之间的关系。     

空间相机像移补偿方法研究

介绍了空间相机拍照时产生像移的机理及国内外目前较常使用的不同像移补偿方法,并对光、机、电等不同实现方法进行分析比较,得出各种方法的优缺点及适用范围。     

防止Ⅱ型驾驶员诱发振荡技术的研究

许多严重的飞行事故都与由速率限制引起的Ⅱ型PIO有关。针对如何预防PIO，首先介绍了自适应杆增益和软件限制环节的设计原理。然后以某带速率限制的电传飞机为例，运用同一理论，分析采用自适应杆增益和软件限制环节来改善速率限制的不利影响。仿真结果表明，自适应杆增益环节和软件限制环节都能抑制住PIO的发生，但两者组合加入抑制效果更好，飞行品质也能达到满意的程度。     

气动谐振管加热振荡流动过程数值研究

为了了解气动谐振管加热现象的振荡流动过程，利用显式TVD－MacCormark格式数值求解二维轴对称雷诺平均N－S方程，获得了一个谐振循环中完整的喷嘴－谐振管系统的振荡流动湍流流场，结果表明，欠膨胀声速冲击喷流固有的流场不均匀性和不稳定性是谐振管加热现象产生的内在原因，激波耗散是谐振管主要的加热机理。     

移相全桥变换器寄生振荡的抑制方法研究

移相全桥变换器是中大功率直流/直流变换场合的一种理想拓扑,但在其输出整流桥上会产生寄生振荡,二极管上存在很高的尖峰电压。这将带来电路损耗并影响整流桥的使用寿命,因此应该想办法抑制。文中分析了寄生振荡产生的原因,介绍了几种可行的抑制方法,并进行了比较研究和实验验证。     

A Possible Transfer Mechanism for the 11-Year Solar Cycle to the Lower Stratosphere

Observational evidence of the 11-year solar cycle (SC) modulation of stratosphere temperatures and winds from the ERA-40 dataset is reviewed, with emphasis on the Northern winter hemisphere. A frequency modulation of sudden warming events is noted, with warmings occurring earlier in solar minimum periods than in solar maximum periods. The observed interaction between the influence of the SC and the quasi biennial oscillation (QBO) on the frequency of sudden warmings is noted as a possible clue for understanding their mechanism of influence. A possible transfer route for the 11-year solar cycle from the equatorial stratopause region to the lowest part of the stratosphere is proposed, via an influence on sudden warming events and the associated induced meridional circulation. SC and QBO composites of zonal wind anomalies show anomalous wind distributions in the subtropical upper stratosphere in early winter. Mechanistic model experiments are reviewed that demonstrate a sensitivity of sudden warmings to small wind anomalies in this region. Various diagnostics from these experiments are shown, including EP fluxes and their divergence and also the synoptic evolution of the polar vortex, in order to understand the mechanism of the influence. Some recent GCM experiments to investigate the SC/QBO interaction are also described. They simulate reasonably well the observed SC/QBO interaction of sudden warming events and appear to support the hypothesis that tropical/subtropical upper stratospheric wind anomalies are an important influence on the timing of sudden warmings.     

高压不稳定环境中的燃料液滴蒸发

对燃料液滴在高压不稳定环境中的蒸发进行了研究，着重讨论了气相介质压力振荡对液滴蒸发特性的影响，计算了Ｃ１２Ｈ２６液滴在Ｎ２介质中蒸发时的蒸发速率、滴温和无因次滴径随时间的变化。结果表明：（１）蒸发速率、滴温发生相同频率的振荡，相位滞后分别为π和π／２；（２）压力振荡使蒸发速率平均值增大，液滴生存时间减少；（３）在不定常加热阶段压力振荡影响很小。     

俯仰振荡三角翼在非定常自由流中运动的实验

在南京航空航天大学已建成的国内首座非定常风洞内,研制了一套单自由度俯仰振荡实验装置,设计开发了一套对模型姿态和来流风速进行联合控制的软件。对一60°后掠三角翼模型进行了单独俯仰振荡运动和俯仰振荡与自由来流耦合运动的实验。实验结果表明:模型做单独俯仰振荡时,振动频率和振动幅值的影响只有在迟滞环出现后才起作用,而迟滞环的出现是由于翼面上的不同流态对外界扰动的反应时间不同造成的。非定常自由流对做俯仰振荡的三角翼气动特性有很大的影响,模型上仰过程中来流的减速,进一步提高了最大升力系数,推迟了失速迎角;模型下俯过程中来流的加速,则更进一步推迟了升力系数恢复到静态时的值。当翼面上产生破碎涡流时,非定常自由流的作用表现得更为明显。     

Observations of a quasi-90-day oscillation in the MLT winds and tides over an equatorial station using meteor radar winds

An evident signature of a least studied quasi-90-day oscillation is found in the winds and tides in the MLT from an equatorial station, São João do Cariri (7.4°S, 36.5°W). The oscillation is found to appear mainly in certain intervals with small but appreciable seasonal (fourth harmonic of annual oscillation) contribution. The maximum amplitude of the oscillation is found to be around 10 m/s in the zonal wind. The enhancement peak of the oscillation exhibits downward movement indicating a plausible role of upward moving waves/tides in carrying its imprint from below to the MLT. Similar oscillation feature in the tropospheric zonal wind and ozone may imply its lower atmospheric origin as a component of the intraseasonal oscillation (ISO) that moves upward by modulating the tides. Subsequently, the propagating tides (mainly semidiurnal) are enhanced by the ozone in the stratosphere through absorption of solar UV radiation and finally manifest the oscillation in the MLT. Consistency of the present findings with the past investigations are observed in some aspects of the oscillation, whereas existing mismatches in others are believed to be due to geophysical variability depending on space and time among various locations on the globe.